Solar System - Contenido educativo - Contenido educativo
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Vídeo subtitulado sobre el Sistema Solar
Our solar system is one of over 500 known solar systems in the entire Milky Way galaxy.
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The solar system came into being about 4.5 billion years ago when a cloud of interstellar gas and dust collapsed,
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resulting in a solar nebula, a swirling disk of material that collided to form the solar system.
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The solar system is located in the Milky Way's Orion star cluster.
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Only 15% of stars in the galaxy host planetary systems, and one of those stars is our own sun.
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Revolving around the sun are eight planets.
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The planets are divided into two categories based on their composition, terrestrial and jovian.
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Terrestrial planets, including Mercury, Venus, Earth, and Mars, are primarily made of rocky material.
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Their surfaces are solid, they don't have ring systems, they have very few or no
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moons, and they are relatively small. The smallest and closest to the Sun is
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Mercury which has the shortest orbit in the solar system at about three Earth
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months. Venus is the hottest planet with temperatures of up to 867 degrees
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Fahrenheit due to an atmosphere of carbon dioxide and extensive lava flows.
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Next to this world of fire is a world of water, Earth.
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The water systems on this planet help create the only known environment in the universe
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capable of sustaining life.
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The last of the terrestrial planets, Mars, might have also supported life about 3.7 billion
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years ago when the planet had a watery surface and moist atmosphere.
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Beyond the four terrestrial planets of the inner solar system lie the Jovian planets
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of the outer solar system.
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The Jovian planets include gas giants Jupiter and Saturn, and ice giants Uranus and Neptune.
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The gas giants are predominantly made of helium and hydrogen, and the ice giants also contain
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rock, ice, and a liquid mixture of water, methane, and ammonia.
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All four Jovian planets have multiple moons, sport ring systems, have no solid surface,
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and are immense.
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The largest Jovian is also the largest planet in the solar system, Jupiter.
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Nearby is Saturn, the solar system's second largest planet.
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Its signature rings are wide enough to fit between Earth and the moon, but are barely
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a kilometer thick.
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Past Saturn are the ice giants Uranus and Neptune.
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The slightly bigger of these ice giants, Uranus, is famous for rotating on its side.
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Next to Uranus is Neptune, the outermost planet in the solar system and also one of the coldest.
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Orbiting the terrestrial planets is the asteroid belt, a flat disk of rocky objects full of
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remnants from the solar system's formation, from microscopic dust particles to the largest
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known object, the dwarf planet Ceres.
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Another disk of space debris lies much further out and orbits the Jovian planets, the icy
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Kuiper Belt.
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Apart from asteroids, the Kuiper Belt is also home to dwarf planets such as Pluto and is
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the birthplace of many comets.
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Beyond the Kuiper Belt is the Oort Cloud, a vast, spherical collection of icy debris.
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It is considered the edge of the solar system since that is where the gravitational and
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physical influences of the Sun end.
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Our solar system's particular configuration of planets and other celestial objects, all
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revolving around a life-giving star make it a special place to call home.
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- Idioma/s:
- Idioma/s subtítulos:
- Autor/es:
- María Luisa González Pascual
- Subido por:
- Maria Luisa G.
- Licencia:
- Reconocimiento - No comercial - Compartir igual
- Visualizaciones:
- 7
- Fecha:
- 26 de junio de 2023 - 19:23
- Visibilidad:
- Clave
- Centro:
- CP INF-PRI LAS ACACIAS
- Duración:
- 04′ 10″
- Relación de aspecto:
- 1.78:1
- Resolución:
- 1280x720 píxeles
- Tamaño:
- 38.03 MBytes